INVESTIGADORES
BERTUCCI Cesar
congresos y reuniones científicas
Título:
Initial Cassini Magnetometer Observations of the neutral sheet of Titan's magnetic tail
Autor/es:
LAW, A. L.; DOUGHERTY, M. K.; MUELLER-WODARG, I. C. F.; BERTUCCI, C. L.; NEUBAUER, F. M.; ARRIDGE, C. S.
Reunión:
Congreso; American Astronomical Society, DPS meeting #37; 2005
Resumen:
Titan is the largest moon of Saturn and the only moon in the solar
system known to have a substantial atmosphere. There is no evidence of
Titan having a significant intrinsic magnetic field, but its atmosphere
does interact with its plasma environment (usually Saturn's
magnetosphere). This interaction results in the magnetic field lines
being draped around Titan, forming a magnetic tail. An important feature
of this magnetic tail is the current carrying neutral sheet, which
separates the Northern and Southern tail lobes. Cassini's first three
close flybys of Titan were all at the same orbital position of 10.5
Saturnian Local Time (SLT) and each time the spacecraft flew through the
neutral sheet plane. The next two flybys observed Titan close to dawn
SLT, where the incident plasma encounters the weaker nightside
ionosphere, again, Cassini flew through the plane of the neutral sheet.
All of these encounters were within Saturn's magnetosphere. In this work
we characterise Titan's neutral sheet as seen by the Cassini
magnetcmeter (MAG) and other Cassini plasma instruments. We comment on
its orientation with respect to the upstream magnetic field and we study
its magnetic structure in order to have an estimate of the amount of
current flowing across this boundary. The implications for the physics
of the structure of the whole magnetic tail will also be discussed.